Eccentric discs in binaries with intermediate mass ratios: Superhumps in the VY Sculptoris stars

Monthly Notices of the Royal Astronomical Society

Volumn 315, Issue 4, 2000, Pages 707-712

  Murray, J R ^b   Warner, B ^a   Wickramasinghe, D T ^c  

^a UNIVERSITY OF CAPE TOWN   (South Africa)

^b UNIVERSITY OF LEICESTER   (United Kingdom)

^c NONE

Author keywords

Accretion, accretion discs; Binaries: close; Hydrodynamics; Instabilities; Methods: numerical; Novae, cataclysmic variables

Indexed keywords

ASTROPHYSICS; STARS;

ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; DISC RADIUS; DISC STRUCTURES; INNER LINDBLAD RESONANCES; MASS RATIO; METHOD: NUMERICAL; NOVAE CATACLYSMIC VARIABLES; SECONDARY STARS;

NUMERICAL METHODS;

EID: 0000709099     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03488.x     Document Type: Article

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